TY - JOUR
T1 - Enhancing searches for astrophysical neutrino sources in IceCube with machine learning and improved spatial modeling
AU - Icecube Collaboration
AU - Schroeder, Frank G.
AU - Bontempo, Federico
AU - Abbasi, R.
AU - Ackermann, M.
AU - Adams, J.
AU - Agarwalla, S. K.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Alameddine, J. M.
AU - Ali, S.
AU - Amin, N. M.
AU - Andeen, K.
AU - Argüelles, C.
AU - Ashida, Y.
AU - Athanasiadou, S.
AU - Axani, S. N.
AU - Babu, R.
AU - Bai, X.
AU - Baines-Holmes, J.
AU - Balagopal, A.
AU - Barwick, S. W.
AU - Bash, S.
AU - Basu, V.
AU - Bay, R.
AU - Beatty, J. J.
AU - Tjus, J. Becker
AU - Behrens, P.
AU - Beise, J.
AU - Bellenghi, C.
AU - Benkel, B.
AU - BenZvi, S.
AU - Berley, D.
AU - Bernardini, E.
AU - Besson, D. Z.
AU - Blaufuss, E.
AU - Bloom, L.
AU - Blot, S.
AU - Bodo, I.
AU - Bontempo, F.
AU - Motzkin, J. Y.Book
AU - Meneguolo, C. Boscolo
AU - Böser, S.
AU - Botner, O.
AU - Böttcher, J.
AU - Braun, J.
AU - Brinson, B.
AU - Brisson-Tsavoussis, Z.
AU - Burley, R. T.
AU - Butterfield, D.
AU - Kiryluk, J.
N1 - Publisher Copyright:
© Copyright owned by the author(s)
PY - 2025/12/30
Y1 - 2025/12/30
N2 - Searches for astrophysical neutrino sources in IceCube rely on an unbinned likelihood that consists of an energy and spatial component. Accurate modeling of the detector, ice, and spatial distributions leads to improved directional and energy reconstructions, resulting in increased sensitivity. In this work, we utilize our best knowledge of the detector ice properties and detector calibrations to reconstruct in-ice particle showers. The spatial component of the likelihood is parameterized either by a 2D Gaussian or a von Mises Fisher (vMF) distribution at small and large angular uncertainties, respectively. Here, we use a gradient-boosted decision tree with a vMF spatial likelihood loss function, reparameterized through two coordinate transformations, to predict per-event point spread functions (PSF). Additionally, we discuss the search for PeV cosmic ray sources using the IceCube Multi-Flavor Astrophysical Neutrino (ICEMAN) sample. Our search contains both an analysis of individual neutrino sources coincident with greater than 100 TeV gamma-ray sources and also a stacking analysis. We outline the prospects for extended neutrino emission originating from the Cygnus Cocoon region.
AB - Searches for astrophysical neutrino sources in IceCube rely on an unbinned likelihood that consists of an energy and spatial component. Accurate modeling of the detector, ice, and spatial distributions leads to improved directional and energy reconstructions, resulting in increased sensitivity. In this work, we utilize our best knowledge of the detector ice properties and detector calibrations to reconstruct in-ice particle showers. The spatial component of the likelihood is parameterized either by a 2D Gaussian or a von Mises Fisher (vMF) distribution at small and large angular uncertainties, respectively. Here, we use a gradient-boosted decision tree with a vMF spatial likelihood loss function, reparameterized through two coordinate transformations, to predict per-event point spread functions (PSF). Additionally, we discuss the search for PeV cosmic ray sources using the IceCube Multi-Flavor Astrophysical Neutrino (ICEMAN) sample. Our search contains both an analysis of individual neutrino sources coincident with greater than 100 TeV gamma-ray sources and also a stacking analysis. We outline the prospects for extended neutrino emission originating from the Cygnus Cocoon region.
UR - https://www.scopus.com/pages/publications/105029010352
U2 - 10.22323/1.501.1169
DO - 10.22323/1.501.1169
M3 - Conference article
AN - SCOPUS:105029010352
SN - 1824-8039
VL - 501
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1169
T2 - 39th International Cosmic Ray Conference, ICRC 2025
Y2 - 15 July 2025 through 24 July 2025
ER -